Preliminary results of new operation mode JULIA Medium Power at JRO

Descripción del Articulo

Poster presented at the 2023 CEDAR Workshop, San Diego, CA, USA, June 25-30
Detalles Bibliográficos
Autores: Kuyeng, Karim, Scipión, Danny, Condor, P., Manay, E., Milla, M.
Formato: objeto de conferencia
Fecha de Publicación:2023
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/5441
Enlace del recurso:http://hdl.handle.net/20.500.12816/5441
Nivel de acceso:acceso abierto
Materia:Equatorial ionosphere
Drifts
JULIA
https://purl.org/pe-repo/ocde/ford#1.05.01
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dc.title.es_ES.fl_str_mv Preliminary results of new operation mode JULIA Medium Power at JRO
title Preliminary results of new operation mode JULIA Medium Power at JRO
spellingShingle Preliminary results of new operation mode JULIA Medium Power at JRO
Kuyeng, Karim
Equatorial ionosphere
Drifts
JULIA
https://purl.org/pe-repo/ocde/ford#1.05.01
title_short Preliminary results of new operation mode JULIA Medium Power at JRO
title_full Preliminary results of new operation mode JULIA Medium Power at JRO
title_fullStr Preliminary results of new operation mode JULIA Medium Power at JRO
title_full_unstemmed Preliminary results of new operation mode JULIA Medium Power at JRO
title_sort Preliminary results of new operation mode JULIA Medium Power at JRO
author Kuyeng, Karim
author_facet Kuyeng, Karim
Scipión, Danny
Condor, P.
Manay, E.
Milla, M.
author_role author
author2 Scipión, Danny
Condor, P.
Manay, E.
Milla, M.
author2_role author
author
author
author
dc.contributor.author.fl_str_mv Kuyeng, Karim
Scipión, Danny
Condor, P.
Manay, E.
Milla, M.
dc.subject.es_ES.fl_str_mv Equatorial ionosphere
Drifts
JULIA
topic Equatorial ionosphere
Drifts
JULIA
https://purl.org/pe-repo/ocde/ford#1.05.01
dc.subject.ocde.es_ES.fl_str_mv https://purl.org/pe-repo/ocde/ford#1.05.01
description Poster presented at the 2023 CEDAR Workshop, San Diego, CA, USA, June 25-30
publishDate 2023
dc.date.accessioned.none.fl_str_mv 2023-08-11T16:40:24Z
dc.date.available.none.fl_str_mv 2023-08-11T16:40:24Z
dc.date.issued.fl_str_mv 2023-06
dc.type.es_ES.fl_str_mv info:eu-repo/semantics/conferenceObject
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dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/5441
url http://hdl.handle.net/20.500.12816/5441
dc.language.iso.es_ES.fl_str_mv eng
language eng
dc.rights.es_ES.fl_str_mv info:eu-repo/semantics/openAccess
dc.rights.uri.es_ES.fl_str_mv https://creativecommons.org/licenses/by-nc-nd/4.0/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-nd/4.0/
dc.format.es_ES.fl_str_mv application/pdf
dc.publisher.es_ES.fl_str_mv 2023 CEDAR Workshop
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spelling Kuyeng, KarimScipión, DannyCondor, P.Manay, E.Milla, M.2023-08-11T16:40:24Z2023-08-11T16:40:24Z2023-06http://hdl.handle.net/20.500.12816/5441Poster presented at the 2023 CEDAR Workshop, San Diego, CA, USA, June 25-30The main radar of the Jicamarca Radio Observatory (JRO), for several years, has operated with two main modes, the ISR mode with big transmitters (1.5 MW), operating around 1000 hours per year, to survey the ionosphere and obtain parameters such as drifts, densities and composition; and the JULIA mode with low power transmitters (20 kW), operating around 4000 hours per year, to measure mostly coherent echoes such as Equatorial Electrojet, Spread F and 150 km echoes to provide with a proxy of the behavior of the ionosphere. Starting in 2022, two new solid-state transmitters were installed at JRO, with peak power of 96 kW each, making it possible to not only detect coherent echoes but to be able to estimate zonal and vertical drifts in the ionosphere too. This new mode, called JULIA Medium Power (JULIA MP), is capable of measuring the same coherent echoes as the original JULIA but able to estimate zonal and vertical drifts up to 500 km. This work will present the preliminary results of this mode, comparisons of the coherent echoes obtained with JULIA and JULIA MP and finally show the quality of drifts we are getting with this medium power mode.application/pdfeng2023 CEDAR Workshopinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-nd/4.0/Equatorial ionosphereDriftsJULIAhttps://purl.org/pe-repo/ocde/ford#1.05.01Preliminary results of new operation mode JULIA Medium Power at JROinfo:eu-repo/semantics/conferenceObjectreponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALPoster_Kuyeng_et_al_2023_CEDAR_Workshop.pdfPoster_Kuyeng_et_al_2023_CEDAR_Workshop.pdfapplication/pdf1166975https://repositorio.igp.gob.pe/bitstreams/ce745ca7-b99b-4f27-917a-f8fcc0f8e626/download5895ddb732e4f4811216484de0c1f10fMD51LICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/b51814fe-3c51-460f-a286-2b11d3cf03a8/download8a4605be74aa9ea9d79846c1fba20a33MD52TEXTPoster_Kuyeng_et_al_2023_CEDAR_Workshop.pdf.txtPoster_Kuyeng_et_al_2023_CEDAR_Workshop.pdf.txtExtracted texttext/plain6116https://repositorio.igp.gob.pe/bitstreams/1577f464-1c68-4a37-9760-cad99284e3a3/download13f37d7bbbd6b1657068a7d1b960a11cMD53THUMBNAILPoster_Kuyeng_et_al_2023_CEDAR_Workshop.pdf.jpgPoster_Kuyeng_et_al_2023_CEDAR_Workshop.pdf.jpgIM Thumbnailimage/jpeg143068https://repositorio.igp.gob.pe/bitstreams/9edbec70-468b-4348-80e5-46123ade6ee0/downloade70957a0e28721bc50e871b280304d08MD5420.500.12816/5441oai:repositorio.igp.gob.pe:20.500.12816/54412023-08-11 16:58:50.279https://creativecommons.org/licenses/by-nc-nd/4.0/info:eu-repo/semantics/openAccessopen.accesshttps://repositorio.igp.gob.peRepositorio Geofísico del Perudspace-help@myu.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Preliminary results of new operation mode JULIA Medium Power at JRO
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